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Chapter 3 Acceleration and free fall - Light and Matter

Chapter 3 Acceleration and free fall - Light and Matter

Chapter 3 Acceleration and free fall - Light and Matter

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Summary<br />

Selected vocabulary<br />

gravity . . . . . . A general term for the phenomenon of attraction<br />

between things having mass. The attraction<br />

between our planet <strong>and</strong> a human-sized object<br />

causes the object to <strong>fall</strong>.<br />

acceleration . . . The rate of change of velocity; the slope of the<br />

tangent line on a v − t graph.<br />

Notation<br />

vo . . . . . . . . . initial velocity<br />

vf . . . . . . . . . final velocity<br />

a . . . . . . . . . . acceleration<br />

g . . . . . . . . . . the acceleration of objects in <strong>free</strong> <strong>fall</strong>; the<br />

strength of the local gravitational field<br />

Summary<br />

114 <strong>Chapter</strong> 3 <strong>Acceleration</strong> <strong>and</strong> <strong>free</strong> <strong>fall</strong><br />

Galileo showed that when air resistance is negligible all <strong>fall</strong>ing<br />

bodies have the same motion regardless of mass. Moreover, their<br />

v − t graphs are straight lines. We therefore define a quantity called<br />

acceleration as the derivative dv/dt. This definition has the advantage<br />

that a force with a given sign, representing its direction, always<br />

produces an acceleration with the same sign. The acceleration of objects<br />

in <strong>free</strong> <strong>fall</strong> varies slightly across the surface of the earth, <strong>and</strong><br />

greatly on other planets.<br />

For motion with constant acceleration, the following three equations<br />

hold:<br />

∆x = vo∆t + 1<br />

2 a∆t2<br />

v 2 f = v2 o + 2a∆x<br />

a = ∆v<br />

∆t<br />

They are not valid if the acceleration is changing.

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